Published December 15, 2004
| Version v1
Journal article
Phenomenology of quintessino dark matter: Production of next lightest supersymmetric particles
- 1. Institute of High Energy Physics, Chinese Academy of Sciences, P.O. Box 918-4, Beijing 100039 (China)
Description
In the model of quintessino as the dark matter particle, the dark matter and dark energy are unified in one superfield, where the dynamics of the Quintessence drives the Universe acceleration and its superpartner, quintessino, makes up the dark matter of the Universe. This scenario predicts the existence of long-lived τ-tilde as the next lightest supersymmetric particle. In this paper we study the possibility of detecting τ-tilde produced by the high energy cosmic neutrinos interacting with the earth matter. By a detailed calculation we find that the event rate is one to several hundred per year at a detector with an effective area of 1 km2. The study in this paper can be also applied to models of gravitino or axino dark matter particles
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.70.123512;
- arXiv
- arXiv:hep-ph/0404263v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 70
- Journal Issue
- 12
- Journal Page Range
- p. 123512-123512.7
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37014223
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- COSMIC NEUTRINOS; COSMOLOGY; NONLUMINOUS MATTER; SPARTICLES; UNIVERSE
- Descriptors DEC
- COSMIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; MATTER; NEUTRINOS; POSTULATED PARTICLES; RADIATIONS
Optional Information
- Notes
- (c) 2004 The American Physical Society